Accretion Processes

Accretion Processes is an astrophysical process in star formation whereby gas and dust from a surrounding molecular cloud or circumstellar disc lose angular momentum and gravitationally infall onto a central protostellar object, thereby governing its mass growth and the dynamical evolution of the protostellar system.

7.2K

Publications

610.7K

Citations

8.4K

Authors

1.7K

Institutions

Publications per year

2017–2026

1.7K

Authors

8.4K

  1. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    63 publications · 11.2K citations

    47

    h-index

  2. RN
    Ramesh Narayan

    Center for Astrophysics Harvard & Smithsonian, United States

    64 publications · 17.4K citations

    47

    h-index

  3. EQ
    Eliot Quataert

    University of California, Berkeley, United States

    47 publications · 4.3K citations

    38

    h-index

  4. DN
    D. N. C. Lin

    University of California, Santa Cruz, United States

    54 publications · 7.8K citations

    38

    h-index

  5. PJ
    Philip J. Armitage

    Joint Institute for Laboratory Astrophysics, United States

    44 publications · 4.5K citations

    35

    h-index

1–5 of 8.4K

Venues

  1. The Astrophysical Journal

    ApJ · 2.2K publications · 218.6K citations

    218

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    1.6K publications · 130.3K citations

    159

    h-index

  3. Astronomy and Astrophysics

    686 publications · 53K citations

    119

    h-index

  4. Nature

    123 publications · 18.9K citations

    73

    h-index

  5. The Astrophysical Journal Letters

    161 publications · 10.4K citations

    58

    h-index

1–5